SDO HMI 2011-06-06 03:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.56 | 183.35 | 19.34 | 97.09 | 9.16 | 336.77 | -18.57 | 62.91 | 0.3546 | -864.0 | -415.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.56 | 7.54 | 339.45 | -15.89 | 63.95 | 0.3034 | -810.0 | -553.8 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 8.12 | 339.14 | -16.20 | 62.67 | 0.3123 | -808.0 | -618.9 | |
| 0.00 | 2.08 | 0.00 | 1.10 | 8.40 | 337.51 | -17.82 | 64.02 | 0.3382 | -834.0 | -604.7 | |
| 2.35 | 148.32 | 1.24 | 78.48 | 9.23 | 337.31 | -18.02 | 62.08 | 0.3471 | -1365.0 | -411.4 | |
| 26.60 | -4.00 | 14.08 | -4.00 | 9.32 | 336.92 | -18.42 | 62.33 | 0.3536 | -1278.2 | 999999 | |
| 1.63 | 1.99 | 0.86 | 1.05 | 8.15 | 336.81 | -18.52 | 65.50 | 0.3470 | -795.4 | -633.5 | |
| 4.89 | 19.27 | 2.59 | 10.21 | 8.24 | 336.32 | -19.01 | 65.80 | 0.3550 | -1032.8 | -748.4 | |
| 1.09 | 2.62 | 0.57 | 1.39 | 7.54 | 336.13 | -19.21 | 67.86 | 0.3536 | 920.5 | 781.8 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 8.15 | 335.90 | -19.43 | 66.49 | 0.3607 | -753.0 | -491.1 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 8.00 | 335.75 | -19.59 | 67.04 | 0.3621 | -651.0 | -461.0 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 9.23 | 333.97 | -21.37 | 65.76 | 0.3960 | -728.0 | -626.0 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 10.19 | 332.97 | -22.36 | 64.53 | 0.4165 | 924.0 | 775.3 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 12.64 | 330.65 | -24.68 | 61.60 | 0.4651 | 893.0 | 741.5 | |
| 0.00 | 0.90 | 0.00 | 0.51 | 13.40 | 329.81 | -25.52 | 60.92 | 0.4815 | 804.0 | 651.3 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |